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Table 1.
Pearson correlation coefficient between the solar asteroseismic age and the solar activity cycle proxy, the 10.7 cm radio emission flux.
| Cycle 23 | Cycle 24 | Two cycles | |
|---|---|---|---|
| GOLF | |||
| BG2, n ≥ 12 | 0.57 ± 0.12 | 0.43 ± 0.12 | 0.50 ± 0.10 |
| BG2, n ≥ 16 | 0.66 ± 0.08 | 0.61 ± 0.09 | 0.60 ± 0.05 |
| BG2, n ≥ 18 | 0.14 ± 0.27 | 0.27 ± 0.19 | 0.25 ± 0.13 |
| K1, n ≥ 12 | 0.69 ± 0.10 | 0.32 ± 0.14 | 0.40 ± 0.02 |
| K1, n ≥ 16 | 0.76 ± 0.05 | 0.35 ± 0.05 | 0.57 ± 0.09 |
| S1, n ≥ 12 | MCMC did not converge | ||
| S1, n ≥ 16 | MCMC did not converge | ||
| BiSON | |||
| BG2, n ≥ 12 | 0.64 ± 0.13 | 0.64 ± 0.11 | 0.65 ± 0.12 |
| BG2, n ≥ 16 | 0.66 ± 0.06 | 0.58 ± 0.07 | 0.67 ± 0.05 |
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